Heating of the Earth. Temperature Layers of the Atmosphere.

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Presentation on theme: "Heating of the Earth. Temperature Layers of the Atmosphere."— Presentation transcript:

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Heating of the Earth

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Temperature Layers of the Atmosphere

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Absorption & Reflection of Solar Energy What is effective at absorbing heat?

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Transfer of Solar Energy  Conduction – energy transferred from one substance to another through direct contact.  Convection – energy transferred from one place to another by the movement of a gas or liquid.

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Heating of the Earth  Does the sun heat the earth evenly?  No, its shape does not allow all places on the surface to receive the same amount of energy.  Which area of the earth receives the most solar energy (heat)?  Equator (most direct sunlight)  Which area of the earth receives the least solar energy?  The poles (least direct sunlight)

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Temperature & Air Pressure  Uneven heating of Earth creates different air pressures (highs and lows).  Air Pressure – Created by the number of air molecules moving and bouncing off an object. (Measured using a barometer.) Examples:  Warm air = more active air molecules = low air pressure –Ex: equator  Cool air = less active air molecules = high air pressure –Ex: poles

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Elevation & Air Pressure

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Air Pressure & Moisture  Low air pressure usually means warm humid weather (ex: equator). Why? –Warm air causes more evaporation; air molecules are more active & can hold more moisture  High air pressure usually means cooler drier weather. Why? –Less evaporation; molecules are close together holding less moisture.

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Differences in Temperature & Air Pressure  Remember: uneven heating of the Earth creates differences in air pressure.  What do the differences in temperature and air pressure create?  Wind  How do they create wind?  Air wants to move from an area of high pressure to an area of low pressure

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Wind Direction

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Sea & Land Breeze Convection Currents

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Global Winds  The uneven heating of the earth creating differences in air pressure creates global winds.  At the poles: indirect solar energy; cold temps; high pressure  air sinks and moves towards the equator.  At the equator: direct solar energy; warm temps; low pressure  air rises and moves towards the poles.  The circular movement is called a convection current.

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Complex Movement of Global Winds  Why isn’t it as simple as one global wind convection current in each the northern & southern hemisphere?  Earth’s rotation affects wind direction.  The influence of the Earth’s rotation on the movement of air and water is called the Coriolis Effect.  The Coriolis Effect cause global winds to turn:  Northern Hemisphere = clockwise  Southern Hemisphere = counter clockwise